Wave propagation in the solar atmosphere

Details Wave propagation in the solar atmosphere Wave propagation in the solar atmosphere

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000kfnts...3..456k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel, Suppl, no. 3, p. 456-457

Physics

Scientific paper

The theory of a wave propagation in the solar atmosphere has been applied to study peculiarities in the wave behaviour above granules and intergranular lanes. We introduced oscillations into a 3D snapshot of the theoretical time dependent solar model atmosphere. NLTE synthesis of the two solar lines was performed: the relatively strong Fe I 5324 Å which is formed over all the photosphere and a weaker Ni I 6768 Å line. The latter is widely used in helioseismology. We compared our modeling with the high spatial resolution observations obtained from the ground using VTT on Tenerife and from space using SOHO/MDI. We conclude that many differences in oscillations above granules and lanes can be induced by variations of the physical conditions in these structures.

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